Results » History » Version 17
Gimenez Silva, Adriana, 12/15/2015 09:36 AM
1 | 15 | PASCHOS, Alexandros | h1. *6. Results* |
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2 | 1 | PASCHOS, Alexandros | |
3 | 1 | PASCHOS, Alexandros | When the communication between the USRPs was established, the transmitted constellation below was obtained. |
4 | 1 | PASCHOS, Alexandros | |
5 | 3 | PASCHOS, Alexandros | p=. !{width: 30%}https://sourceforge.isae.fr/attachments/download/1513/Tx_Constellation.png(Transmitted Constellation)! |
6 | 11 | PASCHOS, Alexandros | _Figure 6.1 Transmitted Constellation_ |
7 | 1 | PASCHOS, Alexandros | |
8 | 16 | Gimenez Silva, Adriana | Using the reshape function in LabVIEW, the symbol rate of 62500 symbols/sec is multiplied by the number of samples per symbol, since the demodulator dunction assumes that this would be the sample rate of the input waveform. The received constellation is shown below. The $BER$ in this case is, evidently, 0. |
9 | 1 | PASCHOS, Alexandros | |
10 | 3 | PASCHOS, Alexandros | p=. !{width: 30%}https://sourceforge.isae.fr/attachments/download/1511/Rx_Constellation_no_noise.png(Received Constellation)! |
11 | 11 | PASCHOS, Alexandros | _Figure 6.2 Received Constellation without AWGN_ |
12 | 1 | PASCHOS, Alexandros | |
13 | 14 | PASCHOS, Alexandros | The constellation on Figure 6.3 was obtained when adding AWGN, for a target $E_b/N_0$ (received $E_b/N_0$) of 5.The constellation will vary as the values of $E_b/N_0$ vary, making it either noisier, or making it resemble a noiseless channel. |
14 | 1 | PASCHOS, Alexandros | |
15 | 3 | PASCHOS, Alexandros | p=. !{width: 30%}https://sourceforge.isae.fr/attachments/download/1512/Rx%20_Constellation_AWGN.png(Noisy Constellation)! |
16 | 11 | PASCHOS, Alexandros | _Figure 6.3 Noisy Constellation_ |
17 | 1 | PASCHOS, Alexandros | |
18 | 16 | Gimenez Silva, Adriana | With AWGN, the $BER$ is calculated, then compared to the theoretical one, obtaining a $BER$ vs $E_b/N_0$ graph like the one depicted below in Figure 6.4. It can be seen that the simulated $BER$ follows, as expected, the same behavior as the theoretical $BER$, validating simulated results |
19 | 1 | PASCHOS, Alexandros | |
20 | 8 | PASCHOS, Alexandros | p=. !{width: 60%}https://sourceforge.isae.fr/attachments/download/1514/BERtheory.jpg(Theroretical an Simulated)! |
21 | 11 | PASCHOS, Alexandros | _Figure 6.4 BER vs Eb/No without coding_ |
22 | 5 | PASCHOS, Alexandros | |
23 | 17 | Gimenez Silva, Adriana | The $BER$ is also calculated for a the BCH code (31,15,3) and for BCH (7,4,1), and compared to the simulated $BER$ without coding. The resulting graphs presented below |
24 | 1 | PASCHOS, Alexandros | |
25 | 17 | Gimenez Silva, Adriana | p=. !{width: 60%}https://sourceforge.isae.fr/attachments/download/1516/BERbch.jpg(BCH Coding(31,15,3))! |
26 | 17 | Gimenez Silva, Adriana | _Figure 6.5 BER vs Eb/No with BCH(31,15,3) coding_ |
27 | 17 | Gimenez Silva, Adriana | |
28 | 17 | Gimenez Silva, Adriana | p=. !{width: 60%}https://sourceforge.isae.fr/attachments/download/1544/BCH%20coding.jpg(BCH Coding BCH(7,4,1))! |
29 | 17 | Gimenez Silva, Adriana | _Figure 6.6 BER vs Eb/No with BCH(7,4,1)_ |
30 | 17 | Gimenez Silva, Adriana | |
31 | 17 | Gimenez Silva, Adriana | Both codes have roughly a rate of 1/2, but it is observed that there is greater improvement for BCH (31, 15,3) since this code can correct more errors in a given bit length (simulated bit stream is of length 3000 bits) than BCH(7,4,1). For BCH (31, 15,3) there is a coding gain of 3,5dB for a $BER=10^-5$ while for BCH(7,4,1) the coding gain for the same $BER$ is of 2dB. |